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In this paper, we have constructed dark energy models in an anisotropicBianchi-V space-time and studied the role of anisotropy in the evolution ofdark energy. We have considered anisotropic dark energy fluid with differentpressure gradients along different spatial directions. In order to obtain adeterministic solution, we have considered three general forms of scale factor.The different forms of scale factors considered here produce time varyingdeceleration parameters in all the cases that simulates the cosmic transition.The variable equation of state (EoS) parameter, skewness parameters for all themodels are obtained and analyzed. The physical properties of the models arealso discussed.

Dark Energy Cosmological Models with General forms of Scale Factor